Abstract
S0 galaxies are key objects for the understanding of galaxy formation not only because they form the link between elliptical and spiral galaxies in the Hubble sequence but, also, because they allow to study the properties of disks unobscured by dust and gas.
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© 1992 Springer Science+Business Media Dordrecht
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Paquet, A., Bender, R., Seifert, W. (1992). Line-Strength Gradients in S0 Galaxies. In: Longo, G., Capaccioli, M., Busarello, G. (eds) Morphological and Physical Classification of Galaxies. Astrophysics and Space Science Library, vol 178. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-2522-2_40
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DOI: https://doi.org/10.1007/978-94-011-2522-2_40
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